Axisymmetric stellar wind models
The effects of stellar rotation on the shape of a star are included in the radiation-driven wind theory in order to study their influence upon disk formation in Be stars. For this purpose, we consider a rotationally oblated star and obtain the line force parameters consistently with the hydrodynamic...
| Publicado: |
2008
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v33_n_p94_Venero http://hdl.handle.net/20.500.12110/paper_14052059_v33_n_p94_Venero |
| Aporte de: |
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